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Dust shell around F and G Main-Sequence stars

✍ Scribed by B. S. Rautela; B. B. Sanwal; G. C. Joshi

Book ID
104866962
Publisher
Springer Netherlands
Year
1990
Tongue
English
Weight
171 KB
Volume
166
Category
Article
ISSN
0004-640X

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The photometer (ISOPHOT) on the Infrared Space Observatory (ISO) has proved to be invaluable for investigating the dust around main sequence stars (both prototypes and candidate Vegalike stars). The long wavelength camera (at 60 and 90 Β΅m) has been used to map the area around the stars to establish